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Spring 1998 Gems & Gemology
VOLUME 34 NO. 1 SPRING 1998 TABLE OF CONTENTS EDITORIAL 1 The Dr. Edward J. Gübelin Most Valuable Article Award FEATURE ARTICLE 4 The Rise to pProminence of the Modern Diamond Cutting Industry in India Menahem Sevdermish, Alan R. Miciak, and Alfred A. Levinson pg. 7 NOTES AND NEW TECHNIQUES 24 Leigha: The Creation of a Three-Dimensional Intarsia Sculpture Arthur Lee Anderson 34 Russian Synthetic Pink Quartz Vladimir S. Balitsky, Irina B. Makhina, Vadim I. Prygov, Anatolii A. Mar’in, Alexandr G. Emel’chenko, Emmanuel Fritsch, Shane F. McClure, Lu Taijing, Dino DeGhionno, John I. Koivula, and James E. Shigley REGULAR FEATURES pg. 30 44 Gem Trade Lab Notes 50 Gem News 64 Gems & Gemology Challenge 66 Book Reviews 68 Gemological Abstracts ABOUT THE COVER: Over the past 30 years, India has emerged as the dominant sup- plier of small cut diamonds for the world market. Today, nearly 70% by weight of the diamonds polished worldwide come from India. The feature article in this issue discuss- es India’s near-monopoly of the cut diamond industry, and reviews India’s impact on the worldwide diamond trade. The availability of an enormous amount of small, low-cost pg. 42 Indian diamonds has recently spawned a growing jewelry manufacturing sector in India. However, the Indian diamond jewelery–making tradition has been around much longer, pg. 46 as shown by the 19th century necklace (39.0 cm long), pendant (4.5 cm high), and bracelet (17.5 cm long) on the cover. The necklace contains 31 table-cut diamond panels, with enamels and freshwater pearls. -
Texas Co-Op Power • March 2017
LOCAL ELECTRIC COOPERATIVE EDITION MARCH 2017 Blizzard of ’57 Spring Vegetable Salads Palo Duro Pageant 35 35on Brake-worthy stops on highway through co-op country THE TRACTOR THAT STARTED IT ALL. IS CHANGING IT ALL. Metal Hood, Fenders New Deluxe Seat** New Swift-TTaach Loader** New Grille Guard New Dash Panel & Operator Platform & Tilt Steering Wheel & Swift-Connect Backhoe & Front Hitch & Display ALL-NEWW KUBOTTAA BX80 SERIES Low-Rate, Long-TTeerm Financing 6 YYeear Goingg On Noww! Limited Powertrain Warrantyy* kubota.com *Only terms and conditions of Kubota’s standard Limited Warranty applyy.. For warranty terms, see Kubota’s Limited Warranty at www.kubota.com or authorized Kubota Dealers. **Only avvaailable on certain models. Optional equipment may be shown. © Kubota TTrractor Corporation, 2017 Since 1944 March 2017 FAVORITES 5 Letters 6 Currents 18 Local Co-op News Get the latest information plus energy and safety tips from your cooperative. 29 Texas History Panhandle Blizzard of 1957 By Dawn Stephens 31 Recipes Spring Vegetable Salads 35 Focus on Texas Photo Contest: In Motion 36 Around Texas List of Local Events 38 Hit the Road Texas on a Grand Stage in Palo Duro By Sheryl Smith-Rodgers Marker near the northern end ONLINE of Interstate 35 in Texas, just TexasCoopPower.com south of the Red River Find these stories online if they don’t appear in your edition of the magazine. FEATURE Texas USA Odessa Meteor Crater 35 on 35 8 Stops with fascinating food, history and popular By E.R. Bills culture lure travelers from the interstate as it weaves Observations through Texas from Mexico to Oklahoma Another Roadside Attraction Story and photos by Julia Robinson By Ryann Ford ROAD TRIP! See video and photos at TexasCoopPower.com NEXT MONTH Drones: An Overview Texas inno- vators, including electric co-ops, hone drones as tools of today. -
Copyrighted Material
Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED -
History of Geology
FEBRUARY 2007 PRIMEFACT 563 (REPLACES MINFACT 60) History of geology Mineral Resources Early humans needed a knowledge of simple geology to enable them to select the most suitable rock types both for axe-heads and knives and for the ornamental stones they used in worship. In the Neolithic and Bronze Ages, about 5000 to 2500 BC, flint was mined in the areas which are now Belgium, Sweden, France, Portugal and Britain. While Stone Age cultures persisted in Britain until after 2000 BC, in the Middle East people began to mine useful minerals such as iron ore, tin, clay, gold and copper as early as 4000 BC. Smelting techniques were developed to make the manufacture of metal tools possible. Copper was probably the earliest metal to be smelted, that is, extracted from its ore by melting. Copper is obtained easily by reducing the green copper carbonate mineral malachite, itself regarded as a precious stone. From 4000 BC on, the use of clay for brick-making became widespread. The Reverend William Branwhite Clarke (1798-1878), smelting of iron ore for making of tools and the ‘father’ of geology in New South Wales weapons began in Asia Minor at about 1300 BC but did not become common in Western Europe until Aristotle believed volcanic eruptions and nearly 500 BC. earthquakes were caused by violent winds escaping from the interior of the earth. Since earlier writers had ascribed these phenomena to The classical period supernatural causes, Aristotle's belief was a By recognising important surface processes at marked step forward. Eratosthenes, a librarian at work, the Greek, Arabic and Roman civilisations Alexandria at about 200 BC, made surprisingly contributed to the growth of knowledge about the accurate measurements of the circumference of earth. -
Replace This with the Actual Title Using All Caps
RADAR POLARIZATION PROPERTIES AND LUNAR SECONDARY CRATERING A Dissertation Presented to the Faculty of the Graduate School of Cornell University In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy by Kassandra Martin-Wells January 2013 © 2013 Kassandra Martin-Wells RADAR POLARIZATION PROPERTIES AND LUNAR SECONDARY CRATERING Kassandra Martin-Wells, Ph. D. Cornell University 2013 Age dating of planetary surfaces relies on an accurate correlation between lunar crater size-frequency distributions and radiometric ages of samples returned from the Moon. For decades, it has been assumed that cratering records are dominated by “primary” impacts of interplanetary bolides [McEwen et al., 2005]. Unlike primary craters, secondary craters, which originate as ejecta from large primary events, occur in large clusters in both space and time. It was long believed that the majority of secondary craters formed at low velocities near their parent crater, resulting in a class of craters with morphologies which are easily distinguished from primary craters of a similar size [McEwen et al., 2005]. However, recent work by Bierhaus et al. (2005), McEwen et al. (2005) argues that cratering records in the Solar System may be strongly contaminated by hard-to-identify secondary craters. They advise caution when relying on counts at small diameters [McEwen et al., 2005; Bierhaus et al., 2005]. Despite the difficulties, something must be done to improve the accuracy of age dates derived from size-frequency distributions of small craters. In this thesis, a method of secondary crater identification based on radar circular polarization properties is presented. The radar polarization and photographic studies of lunar secondary craters in this thesis reveal that secondary cratering is a widespread phenomenon on the lunar surface. -
Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
Warren and Taylor-2014-In Tog-The Moon-'Author's Personal Copy'.Pdf
This article was originally published in Treatise on Geochemistry, Second Edition published by Elsevier, and the attached copy is provided by Elsevier for the author's benefit and for the benefit of the author's institution, for non- commercial research and educational use including without limitation use in instruction at your institution, sending it to specific colleagues who you know, and providing a copy to your institution’s administrator. All other uses, reproduction and distribution, including without limitation commercial reprints, selling or licensing copies or access, or posting on open internet sites, your personal or institution’s website or repository, are prohibited. For exceptions, permission may be sought for such use through Elsevier's permissions site at: http://www.elsevier.com/locate/permissionusematerial Warren P.H., and Taylor G.J. (2014) The Moon. In: Holland H.D. and Turekian K.K. (eds.) Treatise on Geochemistry, Second Edition, vol. 2, pp. 213-250. Oxford: Elsevier. © 2014 Elsevier Ltd. All rights reserved. Author's personal copy 2.9 The Moon PH Warren, University of California, Los Angeles, CA, USA GJ Taylor, University of Hawai‘i, Honolulu, HI, USA ã 2014 Elsevier Ltd. All rights reserved. This article is a revision of the previous edition article by P. H. Warren, volume 1, pp. 559–599, © 2003, Elsevier Ltd. 2.9.1 Introduction: The Lunar Context 213 2.9.2 The Lunar Geochemical Database 214 2.9.2.1 Artificially Acquired Samples 214 2.9.2.2 Lunar Meteorites 214 2.9.2.3 Remote-Sensing Data 215 2.9.3 Mare Volcanism -
Chapter 2 Paleozoic Stratigraphy of the Grand Canyon
CHAPTER 2 PALEOZOIC STRATIGRAPHY OF THE GRAND CANYON PAIGE KERCHER INTRODUCTION The Paleozoic Era of the Phanerozoic Eon is defined as the time between 542 and 251 million years before the present (ICS 2010). The Paleozoic Era began with the evolution of most major animal phyla present today, sparked by the novel adaptation of skeletal hard parts. Organisms continued to diversify throughout the Paleozoic into increasingly adaptive and complex life forms, including the first vertebrates, terrestrial plants and animals, forests and seed plants, reptiles, and flying insects. Vast coal swamps covered much of mid- to low-latitude continental environments in the late Paleozoic as the supercontinent Pangaea began to amalgamate. The hardiest taxa survived the multiple global glaciations and mass extinctions that have come to define major time boundaries of this era. Paleozoic North America existed primarily at mid to low latitudes and experienced multiple major orogenies and continental collisions. For much of the Paleozoic, North America’s southwestern margin ran through Nevada and Arizona – California did not yet exist (Appendix B). The flat-lying Paleozoic rocks of the Grand Canyon, though incomplete, form a record of a continental margin repeatedly inundated and vacated by shallow seas (Appendix A). IMPORTANT STRATIGRAPHIC PRINCIPLES AND CONCEPTS • Principle of Original Horizontality – In most cases, depositional processes produce flat-lying sedimentary layers. Notable exceptions include blanketing ash sheets, and cross-stratification developed on sloped surfaces. • Principle of Superposition – In an undisturbed sequence, older strata lie below younger strata; a package of sedimentary layers youngs upward. • Principle of Lateral Continuity – A layer of sediment extends laterally in all directions until it naturally pinches out or abuts the walls of its confining basin. -
Skempton's Poroelastic Relaxation
Datashare 129 Skempton’s poroelastic relaxation: The mechanism that accounts for the distribution of pore pressure and exhumation-related fractures in black shale of the Appalachian Basin Terry Engelder and Rose-Anna Behr AAPG Bulletin, v. 105, no. 4 (April 2021), pp. 669–694 Copyright ©2021. The American Association of Petroleum Geologists. All rights reserved. EXPLANATIONS FOR TABLE 2: In an expansion of work by Sheldon (1912) on COMPARATIVE TERMINOLOGIES FROM the Appalachian Plateau, east-northeast fractures were SELECTED JOINT STUDIES IN THE mapped across a region large enough to sample rocks APPALACHIAN BASIN through a 20° swing of the Appalachian oroclinal bend (Parker, 1942). Parker (1942) relabeled the strike fi The rst depictions of Appalachian Basin fractures joints in Sheldon (1912) as set III (accompanying paper were in wood block prints by Sarah Hall as they appear Table 2 and in this Datashare). This was necessary ’ in her husband s paper from the geological survey of because the azimuth of these set III joints (i.e., the east- the fourth district of New York (Hall, 1843). A print northeast set) did not follow around the oroclinal of Taughannock Falls cascading over the Geneseo bend as defined by fold axes. Parker (1942, p. 406) black shale a few kilometers north of Ithaca, New York, writes, “Their different character and constant strike shows two major joint sets that are not quite orthogonal. over the whole region point definitely to an indepen- The artist even captured a hint of lithological control dent origin, perhaps simultaneous or perhaps much of the black shale on joint development. -
Naretha Meteorite (Synonyms Kingoonya, Kingooya)
Rec. West. Aust. Mus., 1976, 4 (1) NARETHA METEORITE (Sync;>nyms: Kingoonya, Kingooya) W.H. CLEVERLY* [Received 27 May 1975. Accepted 1 October 1975. Published 31 August 1976.1 ABSTRACT Much of the missing portion of the Naretha (Western Australia) meteorite has been located in museums as an un-named specimen and as two smaller specimens masquerading under the name 'Kingoonya' (or 'Kingooya'). The use of the junior synonyms with their implications of a South Australian site of find should be discontinued. INTRODUCfION Naretha meteorite, an L4 chondrite, was found in 1915 about 3 km north of the 205-mile station during construction of the Trans-Australian Railway. It was broken into at least three major pieces which were acquired by Mr John Darbyshire, Supervising Engineer for the construction of the western end of the railway (construction was proceeding simultaneously from both Kalgoorlie and Port Augusta ends - Fig. 1). Mr Darbyshire donated the meteorite to the W.A. School of Mines in Kalgoorlie where one' piece was retained and exhibited with a photograph of the reassembled meteorite (Fig. 2). A second fragment which was passed on to the Geological Survey of Western Australia was noted briefly by Simpson (1922) who first used the name 'Naretha', the name which had been given to the 205-mile station. There is strong presumptive evidence that the third fragment was passed on to Mr S.F.C. Cook of Kalgoorlie, a private collector from whose inaccurate verbal statements and undocumented collection, the subsequent confusion arose. In late 1926 Mr Cook gave a small piece of 'meteorite to Mr G.W. -
The EERI Oral History Series
CONNECTIONS The EERI Oral History Series Robert E. Wallace CONNECTIONS The EERI Oral History Series Robert E. Wallace Stanley Scott, Interviewer Earthquake Engineering Research Institute Editor: Gail Hynes Shea, Albany, CA ([email protected]) Cover and book design: Laura H. Moger, Moorpark, CA Copyright ©1999 by the Earthquake Engineering Research Institute and the Regents of the University of California. All rights reserved. All literary rights in the manuscript, including the right to publish, are reserved to the Earthquake Engineering Research Institute and the Bancroft Library of the University of California at Berkeley. No part may be reproduced, quoted, or transmitted in any form without the written permission of the executive director of the Earthquake Engi- neering Research Institute or the Director of the Bancroft Library of the University of California at Berkeley. Requests for permission to quote for publication should include identification of the specific passages to be quoted, anticipated use of the passages, and identification of the user. The opinions expressed in this publication are those of the oral history subject and do not necessarily reflect the opinions or policies of the Earthquake Engineering Research Institute or the University of California. Published by the Earthquake Engineering Research Institute 499 14th Street, Suite 320 Oakland, CA 94612-1934 Tel: (510) 451-0905 Fax: (510) 451-5411 E-Mail: [email protected] Web site: http://www.eeri.org EERI Publication No.: OHS-6 ISBN 0-943198-99-2 Library of Congress Cataloging-in-Publication Data Wallace, R. E. (Robert Earl), 1916- Robert E. Wallace / Stanley Scott, interviewer. p. cm – (Connections: the EERI oral history series ; 7) (EERI publication ; no. -
Fire Station Creative Supplementary Submission (699KB Pdf)
FIRE STATION CREATIVE Business Model Overview Background to Organisation Fire Station Creative (FSC) emerged from a voluntary, grassroots organisation whose aim was to find a permanent venue for their arts and cultural activities in Dunfermline. In 2009, they commissioned a feasibility study (£6k), supported by The Big Lottery Fund, to identify a suitable building and demonstrate the public demand for such a proposal. Fife Fire and Rescue Service were scheduled to vacate the old fire station in March 2010. The property was put on the open market by Fife Council that year. Having already viewed the building, the arts group began a campaign through the Dunfermline Press to retain the building in public ownership. After three years, Fife Council changed their position, agreed to lease the building to the arts group and awarded them £170k for the renovation. By this stage the group was now registered as a public charity and operating under the name Fire Station Creative. The Building Renovation The building is currently owned by Fife Council and is category B listed. Completed in 1934, it was designed by renowned Architect, James Shearer, in the classic Art Deco style. It was extended at the rear in the 1980’s and a pitched roof was also added. When Fire Station Creative renovated the building in 2015, the electronic shutters, at the front and rear, were removed and newly designed doors were installed to match the overall aesthetic of the building. Original features were preserved such as the fireman’s poles and the hand painted lettering on the internal doors such as ‘Locker Room’ and ‘Lecture Room’ The entire renovation of the building in 2015 was achieved for around £190k.